Abstract
The Titanium (Ti) isotope compositions of felsic rocks are heavier than their mafic counterparts, and alkaline magmas develop heavier Ti isotope compositions compared to other magma series during magmatic differentiation. Both observations are interpreted to reflect the preferential sequestration of light Ti isotopes in Fe-Ti oxides, such as rutile, ilmenite and titanomagnetite. However, such interpretations so far rely on whole rock studies of cogenetic magmatic samples and the detailed mechanics of oxide-melt equilibrium on the Ti isotope composition of magmas is poorly constrained. To address this, we have measured the Ti isotope composition of co-existing Fe-Ti oxides and groundmass or silicate melt in both natural lavas from contrasting tectonic settings (Heard Island and Santorini), and experimental run products (rutile-melt). All Fe-Ti oxide phases are consistently isotopically lighter than their respective host groundmass or silicate melt, with the magnitude of Δ49/47Tioxide-melt increasing from rutile to ilmenite, and titanomagnetite. The observed difference in Ti isotope fractionation between rutile-melt experiments and ilmenite-groundmass pairs is primarily reflective of small differences in their Tisingle bondO bond length, with ilmenite being isotopically lighter (Δ49/47Tiilmenite-melt extrapolated to 1000 K = −0.600 ± 0.035‰) compared to rutile (Δ49/47Tirutile-melt at extrapolated to 1000 K = −0.404 ± 0.099‰) due to slightly longer Tisingle bondO bonds in ilmenite. In contrast, the variation in Δ49/47Ti observed between titanomagnetite-groundmass pairs increases as a function of increasing TiO2 content (increasing ulvöspinel component) in titanomagnetite, with Δ49/47Tititanomagnetite-melt values extrapolated to 1000 K ranging from −0.811 to −1.451‰ in Ti-rich titanomagnetite (21–23 wt.% TiO2; Usp66-73) from Heard Island compared to −0.673‰ to −0.863 in Santorini (14–15 wt.% TiO2; Usp45-49). We interpret this to result from a weaker and distorted crystal lattice due to changes in the local cationic environment resulting from exchange of smaller Fe3+ ions with larger Fe2+ ions during magnetite-ulvöspinel solid solution. Our results are consistent with fractionation factors inferred from Ti isotopic analyses of mineral separates and ab-initio calculations. We use these fractionation factors in combination with Ti isotope fractionation factors for silicate minerals recalculated from previous studies, along with petrologic information to model the behaviour of Ti isotopes during partial melting of Earth’s mantle as well as reproducing the observed variation in δ49/47Ti of differentiated magmas from distinct geodynamic settings.
| Original language | English |
|---|---|
| Pages (from-to) | 253-272 |
| Number of pages | 20 |
| Journal | Geochimica et Cosmochimica Acta |
| Volume | 326 |
| Early online date | 18 Feb 2022 |
| DOIs | |
| Publication status | E-pub ahead of print - 18 Feb 2022 |
Bibliographical note
Funding Information:The authors gratefully acknowledge Capucine Albert, Max Jansen, Laura Rzehak, and Raúl Fonseca for fruitful discussions. Max Jansen is thanked for assistance with the micro-milling technique, Felipe Leitzke for sharing ab initio data used for VI-fold clinopyroxene fractionation factors, Tony Oldroyd for assistance preparing the samples, and Lindsey Owen for support in the laboratory. The authors would also like to acknowledge detailed and constructive reviews by Sarah Aarons and Paolo Sossi which greatly improved the manuscript. Furthermore, we would like to thank Helen Williams for expert editorial handling. LH acknowledges support from a NERC GW4 + Doctoral Training Partnership studentship (NE/L002434/1). MAM acknowledges support from a NERC standard grant (NE/R001332/1) and a Royal Society Research Grant.
Publisher Copyright:
© 2022 Elsevier Ltd
Keywords
- Titanium isotopes
- Isotope fractionation
- Fractionation factors
- Micro-mill
- Titanomagnetite
- Ilmenite
- Rutile
- Magmatic differentiation
- Mantle melting